Evaluation of solar Type II radio burst estimates of initial solar wind shock speed using a kinematic model of the solar wind on the April 2001 solar event swarm-Reference-Cited by-同舟云学术

Evaluation of solar Type II radio burst estimates of initial solar wind shock speed using a kinematic model of the solar wind on the April 2001 solar event swarm

Published:2002-04 Issue:8 Volume:29 Page:12-1-12-4
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Sun W.¹,Dryer M.²³,Fry C. D.²,Deehr C. S.¹,Smith Z.³,Akasofu S.-I.⁴,Kartalev M. D.⁵,Grigorov K. G.⁵

Affiliation:

1. Geophysical Institute; University of Alaska Fairbanks; Fairbanks Alaska USA

2. Exploration Physics International, Inc.; Milford New Hampshire USA

3. NOAA Space Environment Center; Boulder Colorado USA

4. International Arctic Research Center; University of Alaska Fairbanks; Fairbanks Alaska USA

5. Institute of Mechanics; Bulgarian Academy of Sciences; 1113 Sofia Bulgaria

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference11 articles.

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4. Interplanetary studies: Propagation of disturbances between the Sun and the magnetosphere;Dryer;Space Sci. Rev.,1994

5. Fry , C. D. The three-dimensional geometry of the heliosphere: Quiet time and disturbed periods 1985

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